Theoretical Mechanics - Babeș-Bolyai University

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Lecture 8. Central forces 1 Theoretical Mechanics 10. Central forces. Central forces. Properties (https://people.maths.bris.ac.uk/~marrk/Mech/15_16_CentralF_notes.pdf) A central force is a force acting on a particle of mass m with the property that the force is always directed from m toward, or away, from a fixed point O. The particle is said to move in a central force field. The point O is referred to as the centre of force. Examples: Gravitational force

Transcript of Theoretical Mechanics - Babeș-Bolyai University

Page 1: Theoretical Mechanics - Babeș-Bolyai University

Lecture 8. Central forces 1

Theoretical Mechanics

10. Central forces.

Central forces. Properties (https://people.maths.bris.ac.uk/~marrk/Mech/15_16_CentralF_notes.pdf)

A central force is a force acting on a particle of mass m with the property that

the force is always directed from m toward, or away, from a fixed point O.

The particle is said to move in a central force field. The point O is referred to

as the centre of force. Examples:

Gravitational force

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Lecture 8. Central forces 2

Theoretical Mechanics

Examples:

Coulomb force

Elastic force(spring)

Attractive elastic force

Repulsive elastic force

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Lecture 8. Central forces 3

Theoretical Mechanics

Consider O the center of the force 𝐹 acting on the material point M(m) which

has the position vector 𝑟 = 𝑂𝑀.

Let be

the versor of 𝑟 . Thus, we have

(10.1)

where F is the algebraic

value of 𝐹 .

If F > 0 than 𝐹 is repulsive. Otherwise, if F < 0 than 𝐹 is attractive.

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Theoretical Mechanics

Using the moment of momentum theorem

(10.2)

one obtain the area first integral:

and, thus, the areal velocity is constant.

Remember: Areal velocity (sector velocity, sectorial velocity)

is the rate at which area is swept out by a particle as it

moves along a curve.

The areal velocity of M is:

(10.3)

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Theoretical Mechanics

From (10.2) and (10.3) we have:

In the motion under the action of the central force the moment of momentum

and the areal velocity are constant vectors at any moment 𝑡 ≥ 𝑡0.

(10.4)

We suppose:

Thus, the motion takes place in a plane determined by 𝑟0 and 𝑣 0 (actually the

normal to the plane is ).

From we have and then

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Lecture 8. Central forces 6

Theoretical Mechanics

Next, let us consider the motion of the point M(m) in the plane 𝑂𝑥𝑦 and let be

𝑟, 𝜃 the polar coordinates of the point M.

We have

(10.5)

But, and we obtain :

Equation (10.5) is the area integral (because is the area swept by M)

We have

and it means that

(10.6)

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Lecture 8. Central forces 7

Theoretical Mechanics

Remark. If 𝑐 = 0 then the motion of the point M is rectilinear.

Next we suppose

Taking into account the acceleration form in polar coordinate

(10.7)

Determination of motion in its plane

Consider the motion of the point M(m) in the plane 𝑂𝑥𝑦 and let be 𝑟, 𝜃 the

polar coordinates of the point M. The differential equation of motion is given by

and projecting (10.7) on the polar coordinates versors we obtain:

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Lecture 8. Central forces 8

Theoretical Mechanics

(10.8)

From (10.8)2 we obtain the area first integral

y

x

M0

M

er

e

F

v

O

r r0

v0 α

(10.9)

where

(10.10)

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Lecture 8. Central forces 9

Theoretical Mechanics

From (10.9) we have

And this means that the point M sweeps equal areas in equal intervals of time

(area law).

Thus, the motion of the material the point M

under the action of a central force respect

the area law and takes place in a plane (the

plane motion) determined by the initial

conditions.

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Lecture 8. Central forces 10

Theoretical Mechanics

Case I. 𝑭 = 𝑭(𝒓, 𝜽, 𝒓 , 𝜽 ) (i.e. 𝝏𝑭

𝝏𝒕= 𝟎)

One eliminate time 𝑡 from (10.8)1 by using the area integral (10.9):

Thus, Equation (10.8)1 becomes

(10.11)

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Theoretical Mechanics

When 𝐹 = 𝐹 𝑟, 𝜃 (i.e. The force depends only by position) the equation is as

the Binet‘s equation:

By solving eq. (10.12) one obtain the trajectory of the particle in polar

coordinates. However, in order to solve (10.12) two initial conditions are

necessary. From 𝑟 𝑡0 = 𝑟 0 and 𝑣 𝑡0 = 𝑣 0 we obtain:

(10.12)

(10.13)

Jacques Philippe Marie Binet

(February 2, 1786 – May 12, 1856)

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Indeed,

Thus, we have

y

x

M0

M

er

e

F

v

O

r r0

v0 α

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Lecture 8. Central forces 13

Theoretical Mechanics

Solving (10.12) along with the initial conditions (10.13) one obtain the trajectory

Next, using the area integral r2 𝜃 = 𝑐 we have r2 𝜃 𝑑𝜃 = 𝑐𝑑𝑡 and we obtain:

(10.14)

(10.15)

Now, using (10.14) and (10.16) we get 𝑟 = 𝑟 𝑡 . In this moment the problem is

solved and the motion’s equations in polar coordinates are:

(10.16) and thus

(10.17)

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Theoretical Mechanics

Case II. 𝑭 = 𝑭(𝒓)

In this case it is possible to apply the general theorems of dynamics. First let us

calcuate the elementary work:

Thus, 𝛿𝐿 = 𝐹 𝑟 𝑑𝑟 is an exact differential

and the kinetic energy theorem dT = 𝛿𝐿 = −𝑑𝑉 becomes

𝛿𝐿 = −𝑑𝑉, 𝑉 ≔ − ∫ 𝐹 𝑟 𝑑𝑟

r

rdrrF

mvmvdrF

mvd

0

)(222

2

0

22

(10.18)

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Theoretical Mechanics

Thus,

hdrrFm

v )(22

Energy constant

2

2

22

2

2222

111

rrd

dcv

r

crd

dcr

rrv

We take into account that:

(10.19)

(10.20)

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Theoretical Mechanics

Thus,we have to solve

The energy constant can be calculated from

(10.21) hdrrF

mrrd

dc

)(

2112

2

2

hdrrFm

v )(22

0

(10.22)

Remark. It is also possible to use the Binet‘s equation for the case F=F(r).

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Lecture 8. Central forces 17

Theoretical Mechanics

Example 1.

A particle M(m) moves on a circle of radius b being attracted by a fixed point A

of the circle. Find the attractive force and the velocity of the particle as functions

of r, the distance between M and A.

Solution

Consider the equation of the circle

In polar coordinates we have

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Theoretical Mechanics

Next, in order to obtain the force, we calculate the left hand term of the equation

in order to obtain the force.

),(11

2

2

2

2

rFrrd

d

r

mc

Consider the Binet‘s equation

sign „+“ for repulsive force

sign „–“ for attractive force

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Theoretical Mechanics

Example 2.

Find the motion of a particle M(m=1) that moves under the action of an

attractive force 𝐹 𝑟 =1

𝑟3. At the initial moment we have:

𝑡 = 0: 𝜃0= 0, 𝑟0 = 2, 𝑣0 =1

2, 𝛼 = 𝑟 0, 𝑣 0

=𝜋

4

Solution

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(equation of the trajectory in

polar coordinates, i.e. a

logarithmic spiral)

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Theoretical Mechanics

Using the area law

(equations of motion)

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Theoretical Mechanics

One can use matlab for visualization

t=0:0.01:100;

r=(sqrt(2)*t+4).^(1/2);

theta=(1/2)*log(sqrt(2)/4*t+1);

polar(theta,r)